<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>N.C. Sturchio</dc:contributor>
  <dc:contributor>B. M. Kennedy</dc:contributor>
  <dc:contributor>G.L. Lyon</dc:contributor>
  <dc:contributor>K. Muehlenbachs</dc:contributor>
  <dc:contributor>J.K. Böhlke</dc:contributor>
  <dc:creator>T.A. Abrajano</dc:creator>
  <dc:date>1990</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;Methane-hydrogen gas seeps with mantle-like C and noble gas isotopic characteristics issue from partially serpentinized ultramafic rocks in the Zambales ophiolite, Philippines. New measurements of noble gas and &lt;/span&gt;&lt;sup&gt;14&lt;/sup&gt;&lt;span&gt;C isotope abundances, rock/mixed-volatile equilibrium calculations, and previous chemical and isotopic data suggest that these reduced gases are products of periodotite hydration. The gas seeps are produced in rock-dominated zones of serpentinization, and similar gases may be ubiquitous in ultramafic terranes undergoing serpentinization.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/0883-2927(90)90060-I</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Geochemistry of reduced gas related to serpentinization of the Zambales ophiolite, Philippines</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>